Abstract
| Original language | English |
|---|---|
| Article number | 120601 |
| Pages (from-to) | 1-52 |
| Number of pages | 52 |
| Journal | Physics of Plasmas |
| Volume | 30 |
| Issue number | 12 |
| DOIs | |
| Publication status | Published (in print/issue) - 7 Dec 2023 |
Bibliographical note
Publisher Copyright:© 2023 Author(s).
Data Access Statement
Data sharing is not applicable to this article as no new data were created or analyzed in this study.Funding
Job Beckers acknowledges the financial support from the Dutch Research Council NWO (Project No. 15710). Johannes Berndt and Eva Kovacevic acknowledge the project PEGASUS (Plasma Enabled and Graphene Allowed Synthesis of Unique nano-structures), funded by the European Union’s Horizon research and innovation program under Grant Agreement No. 766894 and the EU Graphene Flagship FLAG-ERA III JTC 2021 project VEGA (No. PR-11938), as well as the support obtained via PERSPECTIVE pubs.aip.org/aip/pop ARD MATEX Region Center, France and project Orleans Metropole, France. Dietmar Block acknowledges funding by the Deutsche Forschungsgemeinschaft (DFG) in Project Nos. BL555 3-2 and BL555 4-2. Peter J. Bruggeman acknowledges the U.S. Department of Energy under Award No. DE-SC-0020232, the National Science Foundation under Award No. PHYS 1903151, and the Army Research Office under Grant No. W911NF-20-1-0105. Lenaïc Couedel acknowledges the support of the Natural Sciences and Engineering Research Council of Canada (NSERC) (Grant No. RGPIN-2019-04333). Gian Luca Delzanno acknowledges the Laboratory Directed Research and Development Program of Los Alamos National Laboratory under Project No. 20230668ER. Los Alamos National Laboratory is operated by Triad National Security, LLC, for the National Nuclear Security Administration of U.S. Department of Energy (Contract No. 89233218CNA000001). Yan Feng acknowledges the support from the National Natural Science Foundation of China (Grant No. 12175159). Ranganathan Gopalakrishnan acknowledges the funding support from U.S. Department of Energy Early Career (Award No. DE-SC0021146) from the Office of Fusion Energy Sciences, U.S. Army Research Office (Award No. W911NF-23-2-0013), and NSF Plasma Physics (Award No. 1903432). Franko Greiner thanks the Deutsche Forschungsgemeinschaf (DFG) for funding of Project No. GR1608/8-1 Dusty plasmas with high electron depletion: Investigation of fundamental mechanisms and properties through particle and plasma diagnostic. Peter Hartmann acknowledges the Hungarian National Office for Research, Development and Innovation (NKFIH) (Grant No. K134462). Mihaly Horanyi acknowledges the NASA Solar System Exploration Research Virtual Research Institute’s (SSERVI), Institute for Modeling Plasmas, Atmospheres, and Cosmic Dust (IMPACT). Christina A. Knapek acknowledges Funding (Grant No. DLR/ BMWiFKZ50WM2161). Uwe Konopka acknowledges that his work was supported by NASA-JPL (Subcontract Nos. 1679198 and 1655063). Uwe Kortshagen acknowledges the support from the Army Research Office under MURI (Grant No. W911NF-18-1-0240) and from the U.S. Department of Energy under Grant No. DESC0022242. Evdokiya G. Kostadinova acknowledges the U.S. National Science Foundation 2694 (Nos. NSF-1903450 and NSF-2308742). Sergei I. Krasheninnikov acknowledges the support of the work by the U.S. Department of Energy, Office of Science, Office of Fusion Energy Sciences under Award No. DE-FG02-06ER54852 at UCSD. I. Mann was supported by the Research Council of Norway through Grant Nos. NFR 275503 and NFR 240065. Davide Mariotti acknowledges EPSRC (Award No. EP/ V055232/1). Lorin Swint Matthews acknowledges the U.S. Department of Energy, Office of Science, Office of Fusion Energy Sciences (Award No. DE-SC-0021334), U.S. Department of Energy Grant No. DESC0021334, NVIDIA Corporation Applied Research Accelerator Program, and the U.S. National Science Foundation (No. NSF1903450). Andre Melzer acknowledges the DLR German Space Agency (50 WM2161 and 50 WM1962). Maxime Mikikian acknowledges the funding (Grant Nos. DLR/BMBF 50WM9852, CNES 02/CNES/4800000059, ANR-11JS09-0010, and ANR-19-CE40-0023). Volodymyr Nosenko, Mikhail Y. Pustylnik, and Hubertus M. Thomas acknowledge the funding (Grant Nos. DLR/BMWi FKZ’s 50WM1441, 50WP1203, 50WP0700, 50WP0203, and 50WP9852). The work of Svetlana Ratynskaia and Panagiotis Tolias has been carried out within the framework of the EUROfusion Consortium, funded by the European Union via the Euratom Research and Training Program (Grant Agreement No. 101052200EUROfusion). Views and opinions expressed are, however, those of the author(s) only and do not necessarily reflect those of the European Union or the European Commission. Neither the European Union nor the European Commission can be held responsible for them. R. Mohan Sankaran acknowledges the U.S. Department of Energy under Grant No. DE-SC0018202 and the Air Force Office of Scientific Research under Grant No. FA9550-19-1-0088. Elijah J. Thimsen acknowledges the financial support from the Army Research Office (ARO) MURI (Grant No. W911NF-18-10240). Edward Thomas, Jr. acknowledges the U.S. Department of Energy (No. SC-0019176) and the U.S. National Science Foundation (No. OIA-2148653).
Keywords
- Condensed Matter Physics
- Phase transitions
- Electrostatics
- Microgravity
- Nanoparticle
- Nuclear fusion
- Aerosols
- Gas discharges
- Plasmas
- Tokomaks